2013ApJ...775L..12T


Query : 2013ApJ...775L..12T

2013ApJ...775L..12T - Astrophys. J., 775, L12 (2013/September-3)

G 10.472+0.027: an extreme water maser outflow associated with a massive protostellar cluster.

TITMARSH A.M., ELLINGSEN S.P., BREEN S.L., CASWELL J.L. and VORONKOV M.A.

Abstract (from CDS):

An Australia Telescope Compact Array search for 22 GHz water masers toward 6.7 GHz class II methanol masers detected in the Methanol Multibeam survey has resulted in the detection of extremely high-velocity emission from one of the sources. The water maser emission associated with this young stellar object covers a velocity span of nearly 300 km/s. The highest velocity water maser emission is redshifted from the systemic velocity by 250 km/s, which is a new record for high-mass star formation regions. The maser is associated with a very young late O, or early B star, which may still be actively accreting matter (and driving the extreme outflow). If that is the case, future observations of the kinematics of this water maser will provide a unique probe of accretion processes in the highest mass young stellar objects and test models of water maser formation.

Abstract Copyright: ∼

Journal keyword(s): infrared: ISM - ISM: molecules - masers - radio lines: ISM - stars: formation

Simbad objects: 10

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Number of rows : 10
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 NGC 3603 OpC 11 14 57.9 -61 14 32           ~ 1136 1
2 3C 279 Bla 12 56 11.16657958 -05 47 21.5251510   18.01 17.75 15.87   ~ 3205 2
3 SSTGLMC G010.4723+00.0272 MIR 18 08 38.226 -19 51 49.98           ~ 1 0
4 MMB G010.472+00.027 cor 18 08 38.2290 -19 51 50.262           ~ 83 1
5 WISE J180838.23-195150.6 MIR 18 08 38.23 -19 51 50.6           ~ 1 0
6 W 31 SFR 18 10 28.6 -19 55 51           ~ 280 0
7 IRAS 18113-2503 pA? 18 14 26.70240 -25 02 55.5792           ~ 34 0
8 W 49n HII 19 10 13.2 +09 06 12           ~ 497 3
9 ICRF J193925.0-634245 Sy2 19 39 25.0245304992 -63 42 45.640373400   18.87 18.37 17.64   ~ 1332 2
10 IRAS 20126+4104 Y*O 20 14 25.8816769656 +41 13 36.879427236           B2.5-B0.5 469 0

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